Two of the most fundamental questions in astrophysics are the conversion of molecular gas into stars and how this physical process is a function of environments...
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ProjectMolecular Gas and Dust in Galaxies Across Cosmic Time
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ProjectMorphology and dynamics of the Milky Way
This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way...
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ProjectMulti-Conjugate Adaptive Optics for EST
IAC is developing a Multi-Conjugate Adaptive Optics (MCAO) bench, with the purpose of demonstrating in laboratory solutions of some of the main problems related...
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ProjectNIRPS (Near Infra Red Planet Searcher)
NIRPS is a next-generation, near-infrared spectrograph that uses adaptive optics and is fed via a fiber link. It is a compact cryogenic Echelle spectrograph...
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ProjectNISP (EUCLID)
The Near Infrared Spectrometer and Photometer (NISP) is an infrared spectrograph for the EUCLID mission. The aim of EUCLID is to obtain a map of the Dark matter...
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ProjectNuclear Activity in Galaxies: a 3D Perspective from the Nucleus to the Outskirts
This project consists of two main research lines. First, the study of quasar-driven outflows in luminous and nearby obscured active galactic nuclei (AGN) and...
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ProjectNucleosynthesis and molecular processes in the late stages of Stellar Evolution
Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch...
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ProjectNuestros Alumnos y el ORM
The LPIYA Group gathers communicators and representatives from every institution present at the Roque de los Muchachos Observatory (ORM), with the objective of...
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ProjectNumerical Astrophysics: Galaxy Formation and Evolution
How galaxies formed and evolved through cosmic time is one of the key questions of modern astronomy and astrophysics. Cosmological time- and length-scales are...